Showing 1–20 of 91 results
/ Date/ Name
Aug 16, 2004HR4049: signature of nova nucleosynthesis ?Apr 15, 2013Decoding the message from meteoritic stardust silicon carbide grainsDec 13, 2011The s process in asymptotic giant branch stars of low metallicity and the composition of carbon-enhanced metal-poor starsAug 29, 2012Short-lived radioactivity in the early Solar System: the Super-AGB star hypothesisAug 9, 2014Stellar origin of the 182Hf cosmochronometer and the presolar history of solar system matterMar 1, 2017Stellar yields and abundances: new directions from planetary nebulaeNov 10, 2025The s Process and BeyondOct 7, 2010Radioactivities in Low- and Intermediate-Mass StarsFeb 16, 2022The RADIOSTAR ProjectAug 3, 2022Origin of Plutonium-244 in the Early Solar SystemOct 1, 2000Advances in s-process modelsJan 22, 2016Origin of the p-process radionuclides 92Nb and 146Sm in the early Solar System and inferences on the birth of the SunMar 2, 2023Representation of s-process abundances for comparison to data from bulk meteoritesSep 24, 2021The stellar beta-decay rate of 134Cs and its impact on the Barium nucleosynthesis in the s processAug 6, 1999Si Isotopic Ratios in Mainstream Presolar SiC Grains RevisitedJun 19, 2020Origin of large meteoritic SiC stardust grains in metal-rich AGB starsSep 11, 2012Can Galactic chemical evolution explain the oxygen isotopic variations in the Solar System?Nov 12, 2013The impact of updated Zr neutron-capture cross sections and new asymptotic giant branch models on our understanding of the s process and the origin of stardustOct 11, 2010Evolution and nucleosynthesis of extremely metal-poor and metal-free low- and intermediate-mass stars II. s-process nucleosynthesis during the core He flashSep 16, 1998A New Astrophysical Interpretation of the Si and Ti Isotopic Compositions of Mainstream SiC Grains from Primitive Meteorites